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Videos de Conceptos Relacionados

Eccentricity of an Ellipse01:27

Eccentricity of an Ellipse

An ellipse is a fundamental conic section defined by the constant sum of distances from any point on its curve to two fixed points, known as the foci. This geometric property can be physically demonstrated using a pencil, string, and two pins. By anchoring the string at both ends and maintaining it taut with a pencil, one can trace the outline of an ellipse.The shape and extent of the ellipse are determined by its eccentricity, e, defined as the ratio of the distance between the center and a...
Atomic Nuclei: Larmor Precession Frequency01:11

Atomic Nuclei: Larmor Precession Frequency

The earth's gravitational field produces a 'twisting force' perpendicular to the angular momentum of a spinning mass (such as a spinning top) that causes the mass to 'wobble' around the gravitational field axis in a phenomenon called precession. Similarly, the magnetic moment (μ) of a spinning nucleus precesses due to an external magnetic field directed along the z-axis. The precession of the magnetic moment vector about the magnetic field is called Larmor precession, and the angular frequency...
Plane Electromagnetic Waves II01:29

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Consider a plane wavefront traveling in position x-direction with a constant speed. This wavefront can be utilized to obtain the relationship between electric and magnetic fields with the help of Faraday's law.
Kepler's Second Law of Planetary Motion01:29

Kepler's Second Law of Planetary Motion

In the early 17th century, German astronomer and mathematician Johannes Kepler postulated three laws for the motion of planets in the solar system. His first law states that all planets orbit the Sun in an elliptical orbit, with the Sun at one of the ellipse's foci. Therefore, the distance of a planet from the Sun varies throughout its revolution around the Sun.
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Galvanometer01:24

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Common devices, including car instrument panels, battery chargers, and inexpensive electrical instruments, measure potential difference (voltage), current, or resistance using a d'Arsonval galvanometer. This electromechanical instrument is also known as a moving coil galvanometer.
The galvanometer consists of  two concave-shaped permanent magnets, providing a uniform radial magnetic field in the annular region. In the center, a pivoted coil of fine copper wire is placed in the uniform magnetic...
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The existence of combined electric and magnetic fields that propagate through space as electromagnetic (EM) waves is the most significant prediction of Maxwell's equations. As Maxwell's equations hold in free space, the predicted electromagnetic waves do not require a medium for their propagation. An EM wave comprises an electric field, defined as the force per charge on a stationary charge, and a magnetic field, which is the force per charge on a moving charge.
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Video Experimental Relacionado

Updated: Jul 5, 2026

A Photonic System for Generating Unconditional Polarization-Entangled Photons Based on Multiple Quantum Interference
07:56

A Photonic System for Generating Unconditional Polarization-Entangled Photons Based on Multiple Quantum Interference

Published on: September 5, 2019

Un pulsar binario milisegundo excéntrico en el plano galáctico.

David J Champion1, Scott M Ransom, Patrick Lazarus

  • 1Department of Physics, McGill University, Montreal, QC H3A 2T8, Canada. David.Champion@atnf.csiro.au

Science (New York, N.Y.)
|May 17, 2008
PubMed
Resumen
Este resumen es generado por máquina.

Los investigadores descubrieron PSR J1903+0327, un púlsar de milisegundos en una órbita inusual con un compañero de masa solar. Este hallazgo desafía los modelos convencionales de la evolución de las estrellas binarias y la formación de púlsares.

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Área de la Ciencia:

  • La astronomía y la astrofísica.
  • Objetos compactos Objetos compactos.
  • Los sistemas binarios son sistemas binarios.

Sus antecedentes:

  • Los sistemas de púlsares binarios son cruciales para comprender la evolución estelar y la física extrema.
  • Los púlsares de milisegundos (MSP) son estrellas de neutrones que giran rápidamente.

Objetivo del estudio:

  • Para investigar las propiedades de un pulsar de radio recién descubierto, PSR J1903+0327.
  • Para entender sus inusuales características orbitales y su estrella compañera.

Principales métodos:

  • Realizó una encuesta utilizando el telescopio de Arecibo para detectar pulsares de radio.
  • Realizó observaciones infrarrojas para identificar la estrella compañera.
  • Analizó las observaciones de cronometraje de pulsares utilizando métodos relativistas.

Principales resultados:

  • Descubrió PSR J1903+0327, un púlsar de milisegundos con un período de 2,15 ms.
  • Se observó una órbita muy excéntrica (e=0.44) de 95 días alrededor de un compañero de masa solar.
  • Identificó una posible estrella compañera de la secuencia principal.
  • Se determinó una masa pulsar inusualmente alta de 1,74 ± 0,04 masas solares.

Conclusiones:

  • El sistema observado desafía los modelos convencionales de evolución estelar binaria.
  • Se proponen escenarios de formación alternativos, como la eyección de cúmulos globulares o triples jerárquicos.
  • La gran masa sugiere una formación única o vías evolutivas para este púlsar.